Science Source Feb 2010

EN_90286391_0226

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caption

Solar eclipse sequence shot at 7 minute intervals. The sequence shows the disc of the Moon gradually moving over the disc of the Sun, and then moving away again. At totality, the Moon fits perfectly over the Sun and the corona (white), the Sun's atmosphere, becomes visible. It is not visible at other times because of the overwhelming brightness of the rest of the Sun. The moment of totality lasts for only a few minutes. Total solar eclipses usually occur less than once a year, and can only be seen from a small area of the Earth's surface.

headline Science Source Feb 2010

created date 2010-02-13

credit EAST NEWS

source Science Source

byline Science Source

original transmission reference 4h8929

weight 0,78MB

size 28cm x 19cm by 300dpi

keywords - Show

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